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THE GALAXY UV LUMINOSITY FUNCTION BEFORE THE EPOCH OF REIONIZATION

  • Authors: Charlotte A. Mason, Michele Trenti, and Tommaso Treu

2015 The Astrophysical Journal 813 21.

  • Provider: AAS Journals

Caption: Figure 4.

Contribution to predicted UV luminosity from the 0th and 1st order terms in Equation (3) as a function of observed redshift for fixed halo mass, Mh = 1011 M. The contribution from star formation during the halo assembly time (solid) dominates, with the contribution from the earlier star formation epoch (dashed) increasing with redshift. The SFR is constant in both epochs.

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